Built on

M. Schmidt, The Rate of Star Formation
1959
Earlier work this paper cites.
J. I. Castor, Spectral line formation in Wolf-Rayet envelopes
1970
Earlier work this paper cites.
P. Goldreich and J. Kwan, Molecular Clouds
1974
Earlier work this paper cites.
R. H. Hildebrand, The Determination of Cloud Masses and Dust Characteristics from Submillimetre Thermal Emission
1983
Earlier work this paper cites.
R. C. Kennicutt, Jr., The star formation law in galactic disks
1989
Earlier work this paper cites.
Z. Haiman, A. A. Thoul, and A. Loeb, Cosmological Formation of Low-Mass Objects
1996
Earlier work this paper cites.
P. Madau, A. Meiksin, and M. J. Rees, 21 Centimeter Tomography of the Intergalactic Medium at High Redshift
1997
Earlier work this paper cites.
M. Tegmark, J. Silk, M. J. Rees, A. Blanchard, T. Abel, and F. Palla, How Small Were the First Cosmological Objects?
1997
Earlier work this paper cites.
H. J. Mo, S. Mao, and S. D. M. White, The formation of galactic discs
1998
Earlier work this paper cites.
R. C. Kennicutt, Jr., The Global Schmidt Law in Star-forming Galaxies
1998
Earlier work this paper cites.
M. Suginohara, T. Suginohara, and D. N. Spergel, Detecting z > > 10 Objects through Carbon, Nitrogen, and Oxygen Emission Lines
1999
Earlier work this paper cites.
R. K. Sheth and G. Tormen, Large-scale bias and the peak background split
1999
Earlier work this paper cites.
L. Dunne, S. Eales, M. Edmunds, R. Ivison, P. Alexander, and D. L. Clements, The SCUBA Local Universe Galaxy Survey - I. First measurements of the submillimetre luminosity and dust mass functions
2000
Earlier work this paper cites.
P. F. Goldsmith, Molecular Depletion and Thermal Balance in Dark Cloud Cores
2001
Earlier work this paper cites.
H. J. Mo and S. D. M. White, The abundance and clustering of dark haloes in the standard Λ \Lambda CDM cosmogony
2002
Earlier work this paper cites.
A. Loeb and M. Zaldarriaga, Measuring the Small-Scale Power Spectrum of Cosmic Density Fluctuations through 21cm Tomography Prior to the Epoch of Structure Formation
2004
Earlier work this paper cites.
M. Zaldarriaga, S. R. Furlanetto, and L. Hernquist, 21 Centimeter Fluctuations from Cosmic Gas at High Redshifts
2004
Earlier work this paper cites.
P. B. Alton, E. M. Xilouris, A. Misiriotis, K. M. Dasyra, and M. Dumke, The emissivity of dust grains in spiral galaxies
2004
Earlier work this paper cites.
S. R. Furlanetto, S. P. Oh, and F. H. Briggs, Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe
2006
Earlier work this paper cites.

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P. Chanial, H. Flores, B. Guiderdoni, D. Elbaz, F. Hammer, and L. Vigroux, The infrared compactness-temperature relation for quiescent and starburst galaxies
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Then

F. Mannucci, R. Salvaterra, and M. A. Campisi, The metallicity of the long GRB hosts and the fundamental metallicity relation of low-mass galaxies
Original
2011
Later among the works it cites.
R. Davies, D. Mark, and A. Sternberg, Dense molecular gas around AGN: HCN/CO in NGC 3227
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Later among the works it cites.
A. R. Pullen, T.-C. Chang, O. Doré, and A. Lidz, Cross-correlations as a Cosmological Carbon Monoxide Detector
Original
2013
Later among the works it cites.
J. A. Muñoz and S. R. Furlanetto, Molecular cloud properties and CO line emission in z > > 6 galaxies
Original
2013
Later among the works it cites.
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2015

Predicting the intensity mapping signal for multi-$J$ CO lines

Mashian, Natalie, Sternberg, Amiel, Loeb, Abraham

Understand

We present a novel approach to estimating the intensity mapping signal of any CO rotational line emitted during the Epoch of Reionization (EoR).

Our approach is based on large velocity gradient (LVG) modeling, a radiative transfer modeling technique that generates the full CO spectral line energy distribution (SLED) for a specified gas kinetic temperature, volume density, velocity gradient, molecular abundance, and column density.
These parameters, which drive the physics of CO transitions and ultimately dictate the shape and amplitude of the CO SLED, can be linked to the global properties of the host galaxy, mainly the star formation rate (SFR) and the SFR surface density.
By further employing an empirically derived SFR-M relation for high redshift galaxies, we can express the LVG parameters, and thus the specific intensity of any CO rotational transition, as functions of the host halo mass M and redshift z.

Built on

M. Schmidt, The Rate of Star Formation
1959
Earlier work this paper cites.
J. I. Castor, Spectral line formation in Wolf-Rayet envelopes
1970
Earlier work this paper cites.
P. Goldreich and J. Kwan, Molecular Clouds
1974
Earlier work this paper cites.
R. H. Hildebrand, The Determination of Cloud Masses and Dust Characteristics from Submillimetre Thermal Emission
1983
Earlier work this paper cites.
R. C. Kennicutt, Jr., The star formation law in galactic disks
1989
Earlier work this paper cites.
Z. Haiman, A. A. Thoul, and A. Loeb, Cosmological Formation of Low-Mass Objects
1996
Earlier work this paper cites.
P. Madau, A. Meiksin, and M. J. Rees, 21 Centimeter Tomography of the Intergalactic Medium at High Redshift
1997
Earlier work this paper cites.
M. Tegmark, J. Silk, M. J. Rees, A. Blanchard, T. Abel, and F. Palla, How Small Were the First Cosmological Objects?
1997
Earlier work this paper cites.
H. J. Mo, S. Mao, and S. D. M. White, The formation of galactic discs
1998
Earlier work this paper cites.
R. C. Kennicutt, Jr., The Global Schmidt Law in Star-forming Galaxies
1998
Earlier work this paper cites.
M. Suginohara, T. Suginohara, and D. N. Spergel, Detecting z > > 10 Objects through Carbon, Nitrogen, and Oxygen Emission Lines
1999
Earlier work this paper cites.
R. K. Sheth and G. Tormen, Large-scale bias and the peak background split
1999
Earlier work this paper cites.
L. Dunne, S. Eales, M. Edmunds, R. Ivison, P. Alexander, and D. L. Clements, The SCUBA Local Universe Galaxy Survey - I. First measurements of the submillimetre luminosity and dust mass functions
2000
Earlier work this paper cites.
P. F. Goldsmith, Molecular Depletion and Thermal Balance in Dark Cloud Cores
2001
Earlier work this paper cites.
H. J. Mo and S. D. M. White, The abundance and clustering of dark haloes in the standard Λ \Lambda CDM cosmogony
2002
Earlier work this paper cites.
A. Loeb and M. Zaldarriaga, Measuring the Small-Scale Power Spectrum of Cosmic Density Fluctuations through 21cm Tomography Prior to the Epoch of Structure Formation
2004
Earlier work this paper cites.
M. Zaldarriaga, S. R. Furlanetto, and L. Hernquist, 21 Centimeter Fluctuations from Cosmic Gas at High Redshifts
2004
Earlier work this paper cites.
P. B. Alton, E. M. Xilouris, A. Misiriotis, K. M. Dasyra, and M. Dumke, The emissivity of dust grains in spiral galaxies
2004
Earlier work this paper cites.
S. R. Furlanetto, S. P. Oh, and F. H. Briggs, Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe
2006
Earlier work this paper cites.